Nonlinear MHD simulations of tidally excited waves show that a strong initial magnetic dipole suppresses zonal flows and restores linear tidal dissipation, while a weak field allows flows to reshape the field and nonlinear dissipation.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Interactions between tidal flows and magnetic fields in stellar/planetary convective envelopes
Nonlinear MHD simulations of tidally excited waves show that a strong initial magnetic dipole suppresses zonal flows and restores linear tidal dissipation, while a weak field allows flows to reshape the field and nonlinear dissipation.